Chris Smith

UCHIME improves sensitivity and speed of chimera detection

NGC 6240: merger-induced star formation and gas dynamics

On the relation of optical obscuration and X-ray absorption in Seyfert galaxies

A catalogue of quasars and active nuclei: 13th edition

A catalogue of quasars and active nuclei: 12th edition

First simultaneous NIR/X-ray detection of a flare from Sgr A*

Strategies for improving the sustainability of structural metals

A Stepwise Huisgen Cycloaddition Process: Copper(I)-Catalyzed Regioselective “Ligation” of Azides and Terminal Alkynes

Click Chemistry In Situ: Acetylcholinesterase as a Reaction Vessel for the Selective Assembly of a Femtomolar Inhibitor from an Array of Building Blocks

Within-subject template estimation for unbiased longitudinal image analysis

A review of statistically-based landslide susceptibility models

Vision-based material recognition for automated monitoring of construction progress and generating building information modeling from unordered site image collections

Construction of Interlocking and Threaded Rings Using Two Different Transition Metals as Templating and Connecting Centers:  Catenanes and Rotaxanes Incorporating Ru(terpy)₂-Units in Their Framework

Status of R&D activities on materials for fusion power reactors

A new type of catenand: Interlocked macrocycles held together by intramolecular sandwich benzo-15-crown-5 potassium complexes

Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution

Irreversible but Noncovalent Ru(II)−Pyridine Bond:  Its Use for the Formation of [2]-Catenanes

Prospects of CO₂ Utilization via Direct Heterogeneous Electrochemical Reduction

Building Information Modeling (BIM) for existing buildings — Literature review and future needs

Areas beneath the relative operating characteristics (ROC) and relative operating levels (ROL) curves: Statistical significance and interpretation

Current State of Development of Electricity-Generating Technologies: A Literature Review

Will Jets Identify the Progenitors of Type I[CLC]a[/CLC] Supernovae?

SHINING, A Survey of Far-infrared Lines in Nearby Galaxies. I. Survey Description, Observational Trends, and Line Diagnostics

The Deepest Supernova Search is Realized in the Hubble Ultra Deep Field Survey

Structural materials for fission & fusion energy

The X-Ray-to-Optical Properties of Optically Selected Active Galaxies over Wide Luminosity and Redshift Ranges

Click Chemistry In Situ: Acetylcholinesterase as a Reaction Vessel for the Selective Assembly of a Femtomolar Inhibitor from an Array of Building Blocks

Assessment of Eco-friendly Gases for Electrical Insulation to Replace the Most Potent Industrial Greenhouse Gas SF₆

f(R,T)gravity

Advanced materials for fusion technology

Chandra Multiwavelength Project. I. First X‐Ray Source Catalog

Current Challenges and Perspectives in Resistive Gaseous Detectors: a manifesto from RPC 2012

The farthest known supernova: Support for an accelerating universe and a glimpse of the \nepoch of deceleration

First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Determination of Cosmological Parameters

Recognition-mediated regiocontrol of a dipolar cycloaddition reaction

The access principle: the case for open access to research and scholarship

Imaged-based verification of as-built documentation of operational buildings

The Magnification of SN 1997[CLC]ff[/CLC], the Farthest Known Supernova

Recent Developments in Irradiation-Resistant Steels

Materials challenges in nuclear energy

The Expected Properties of Dark Lenses

The Luminous Type Ic Supernova 1992ar at z = 0.145

The Chandra Multi‐wavelength Project (ChaMP): Results and prospects

ChandraObservations of the QSO Pair Q2345+007: Binary or Massive Dark Lens?

The path to fusion power

The Luminous Type Ic Supernova 1992ar at \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $z=0.145$ \end{document}

The need for fusion

Benzo-15-crown-5 derivatives. Synthesis and properties as ion-extraction and ion-transport agents

The Large Hadron Collider: lessons learned and summary

Fusion

Discovery of a [CLC][ITAL]z[/ITAL][/CLC] = 4.93, X-Ray–selected Quasar by the [ITAL]Chandra[/ITAL] Multiwavelength Project (C[CLC]ha[/CLC]MP)

The Large Hadron Collider